On the benefits of photometry for roAp theory: MOST observations of γ Equulei (HD 201601)

Details On the benefits of photometry for roAp theory: MOST observations of γ Equulei (HD 201601) On the benefits of photometry for roAp theory: MOST observations of γ Equulei (HD 201601)

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coska..38..311g&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2, p. 311-316.

Astronomy and Astrophysics

Astronomy

Stars: Chemically Peculiar, Stars: Oscillation, Methods: Observational, Techniques: Space Photometry

Scientific paper

We discuss the potential of space photometry for rapidly oscillating Ap (roAp) stars. In reference to the MOST observations of γEquulei (Gruberbauer et al., 2008), we show that several aspects of the roAp phenomenon demand longer observational time bases and better time sampling than those currently feasible using spectroscopy. We conclude that, in order to improve our understanding of roAp stars, photometry is still an important tool which should not be neglected.

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